Submissions from 2023
The Gas and Stellar Content of a Metal-poor Galaxy at z = 8.496 as Revealed by JWST and ALMA, K. E. Heintz, C. Giménez-Arteaga, S. Fujimoto, Gabriel B. Brammer, D. Espada, S. Gillman, J. González-López, T. R. Greve, Yuichi Harikane, B. Hatsukade, K. K. Knudsen, Anton M. Koekemoer, K. Kohno, V. Kokorev, M. M. Lee, Georgios E. Magdis, E. J. Nelson, F. Rizzo, Ryan L. Sanders, D. Schaerer, Alice E. Shapley, V. B. Strait, S. Toft, F. Valentino, A. van der Wel, A. P. Vijayan, D. Watson, F. E. Bauer, Amber Christiansen, C. R. Christiansen, and S. N. Wilson
Gauging the mass of metals in the gas phase of galaxies from the Local Universe to the Epoch of Reionization, K. E. Heintz, Alice E. Shapley, Ryan L. Sanders, M. Killi, D. Watson, G. Magdis, F. Valentino, M. Ginolfi, D. Narayanan, T. R. Greve, J. P. U. Fynbo, D. Vizgan, and S. N. Wilson
Early Results from GLASS–JWST. XXI. Rapid Asembly of a Galaxy at z = 6.23 Revealed by Its C/O Abundance, Tucker Jones, Ryan L. Sanders, Yuguang Chen, Xin Wang, Takahiro Morishita, Guido Roberts-Borsani, Tommaso Treu, Alan Dressler, Emiliano Merlin, Diego Paris, Paola Santini, Pietro Bergamini, A. Henry, Erin Huntzinger, Themiya Nanayakkara, Kristan Boyett, Marusa Bradac, Gabriel B. Brammer, Antonello Calabró, Karl Glazebrook, Kathryn Grasha, Sara Mascia, Laura Pentericci, Michele Trenti, and Benedetta Vulcani
Exclusive J/𝜓 detection and physics with ECCE, X. Li
An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in 1.3 <= z <= 2.6 Star-forming Galaxies from MOSDEF, Brian Lorenz, Mariska Kriek, Alice E. Shapley, Naveen Reddy, Ryan L. Sanders, Guillermo Barro, Alison L. Coil, Bahram Mobasher, Sedona H. Price, Jordan N. Runco, Irene Shivaei, Brian Siana, and Daniel R. Weisz
The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques, Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher, Elisabete da Cunha, Viviana Acquaviva, Denis Burgarella, Gabriela Calistro Rivera, Adam C. Carnall, Yu-Yen Chang, Nima Chartab, Kevin C. Cooke, Ciaran Fairhurst, Jeyhan Kartaltepe, Joel Leja, Katarzyna Małek, Brett Salmon, Marianna Torelli, Alba Vidal-García, Médéric Boquien, Gabriel B. Brammer, Michael J. I. Brown, Peter L. Capak, Jacopo Chevallard, Chiara Circosta, Darren Croton, Iary Davidzon, Mark Dickinson, Kenneth J. Duncan, Sandra M. Faber, Harry C. Ferguson, Adriano Fontana, Yicheng Guo, Boris Haeussler, Shoubaneh Hemmati, Marziye Jafariyazani, Susan A. Kassin, Rebecca L. Larson, Bomee Lee, Kameswara Bharadwaj Mantha, Francesca Marchi, Hooshang Nayyeri, Jeffrey A. Newman, Viraj Pandya, Janine Pforr, Naveen Reddy, Ryan L. Sanders, Ekta Shah, Abtin Shahidi, Matthew L. Stevans, Dian Puspita Triani, Krystal D. Tyler, Brittany N. Vanderhoof, Alexander de la Vega, Weichen Wang, and Madalyn E. Weston
The dust-to-gas mass ratio of luminous galaxies as a function of their metallicity at cosmic noon, Gergö Popping, Irene Shivaei, Ryan L. Sanders, Tucker Jones, Alexandra Pope, Naveen Reddy, Alice E. Shapley, Alison L. Coil, and Mariska Kriek
The Impact of Star-formation-rate Surface Density on the Electron Density and Ionization Parameter of High-redshift Galaxies, Naveen Reddy, Ryan L. Sanders, Alice E. Shapley, Michael W. Topping, Mariska Kriek, Alison L. Coil, Bahram Mobasher, Brian Siana, and Saeed Rezaee
A JWST/NIRSpec Exploration of the Connection between Ionization Parameter, Electron Density, and Star-formation-rate Surface Density in z = 2.7–6.3 Galaxies, Naveen Reddy, Michael W. Topping, Ryan L. Sanders, Alice E. Shapley, and Gabriel B. Brammer
Paschen-line Constraints on Dust Attenuation and Star Formation at z ∼ 1–3 with JWST/ NIRSpec, Naveen Reddy, Michael W. Topping, Ryan L. Sanders, Alice E. Shapley, and Gabriel B. Brammer
A Preview of JWST Metallicity Studies at Cosmic Noon: The First Detection of Auroral [O II] Emission at High Redshift, Ryan L. Sanders, Alice E. Shapley, Leonardo Clarke, Michael W. Topping, Naveen Reddy, Mariska Kriek, Tucker Jones, Daniel P. Stark, and Mengtao Tang
CO Emission, Molecular Gas, and Metallicity in Main-sequence Star-forming Galaxies at z ∼ 2.3, Ryan L. Sanders, Alice E. Shapley, Tucker Jones, Irene Shivaei, Gergö Popping, Naveen Reddy, Romeel Davé, Sedona H. Price, Bahram Mobasher, Mariska Kriek, Alison L. Coil, and Brian Siana
Excitation and Ionization Properties of Star-forming Galaxies at z = 2.0-9.3 with JWST/NIRSpec, Ryan L. Sanders, Alice E. Shapley, Michael W. Topping, Naveen Reddy, and Gabriel B. Brammer
ECCE sensitivity studies for single hadron transverse single spin asymmetry measurements, R. Seidl, A. Vladimirov, D. Pitonyak, and A. Prokudin
JWST/NIRSpec Measurements of the Relationships between Nebular Emission-line Ratios and Stellar Mass at z ∼ 3–6, Alice E. Shapley, Naveen Reddy, Ryan L. Sanders, Michael W. Topping, and Gabriel B. Brammer
JWST/NIRSpec Balmer-line Measurements of Star Formation and Dust Attenuation at z ∼ 3–6, Alice E. Shapley, Ryan L. Sanders, Naveen Reddy, Michael W. Topping, and Gabriel B. Brammer
Azimuthal anisotropy measurement of (multi)strange hadrons in Au+Au collisions at √𝑠𝑁𝑁=54.4 GeV, STAR Collaboration
Azimuthal anisotropy measurement of (multi)strange hadrons in Au+Au collisions at √s NN = 54.4 GeV, STAR Collaboration
Beam Energy Dependence of Fifth- and Sixth-Order Net-Proton Number Fluctuations in Au + Au Collisions at RHIC, STAR Collaboration
Beam Energy Dependence of Fifth- and Sixth-Order Net-Proton Number Fluctuations in Au + Au Collisions at RHIC, STAR Collaboration
Beam energy dependence of the linear and mode-coupled flow harmonics in Au+Au collisions, STAR Collaboration
Global polarization of Λ and Λ¯ hyperons in Au+Au collisions at √s NN = 19.6 and 27 GeV, STAR Collaboration
K∗0 production in Au + Au collisions at √sNN = 7.7, 11.5, 14.5, 19.6, 27, and 39 GeV from the RHIC beam energy scan, STAR Collaboration
Measurement of Sequential ϒ Suppression in Au + Au Collisions at √sNN = 200 GeV with the STAR Experiment, STAR Collaboration
Measurements of dielectron production in Au + Au collisions at √sNN = 27, 39, and 62.4 GeV from the STAR experiment, STAR Collaboration
